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Validation of the Electromagnetic Physical Processes with Software SPENVIS

Received: 16 September 2015    Accepted: 13 October 2015    Published: 27 October 2015
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Abstract

The Space Radiation represents a serious risk for astronauts during space missions. The risk related to the space radiation exposure could involve acute and/or late effects. The Solar Cosmic Radiation that consists of protons (≈98%) with a very wide spectrum in energy (up to several GeV), is the major source of exposure for the crew. In this paper we present the results of the validation of the electromagnetic physical processes with the aim to contribute to the study of radiation protection for astronauts, in particular against the radiation due to the Solar Particle Events (SPE). The simulation was performed using MULASSIS, a module to the software SPENVIS, with protons as source, in the energy range from 800 MeV to 1.2 GeV, on a slab of aluminum of mass thickness of 20 g/cm2. The results obtained by the simulation were compared with PSTAR database of the NIST. Finally, a comparison between SPENVIS and Geant4-9.6p2 was performed.

Published in American Journal of Environmental Protection (Volume 4, Issue 6)
DOI 10.11648/j.ajep.20150406.12
Page(s) 275-278
Creative Commons

This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.

Copyright

Copyright © The Author(s), 2024. Published by Science Publishing Group

Keywords

Space Radiation, SPENVIS-MULASSIS, Geant4, Protons, Al Target

References
[1] S. Agostinelli, J. Allison, K. Amako, J. Apostolakis, et al., Geant4 - A simulation toolkit. Nucl. Instrum, Meth. Phys. Res. A506 (3), 250-303, 2003.
[2] K. Amako, S. Guatelli, V. N. Ivanchenko, M. Maire, B. Mascialino, K. Murakami, P. Nieminen, L. Pandola, S. Parlati, M. G. Pia, M. Piergentili, T. Sasaki, and L. Urban, Comparison of Geant4 Electromagnetic Physics Models Against the NIST Reference Data, IEEE Trans. Nuc. Sci, Vol 52 (2005).
[3] M. J. Berger, ESTAR, PSTAR, and ASTAR: Computer Programs for Calculating Stopping-Power and Range Tables for Electrons, Protons, and Helium Ions (version 1.2.3), National Institute of Standards and Technology, Gaithersburg, MD., [Online] 2005. Available: http://physics.nist.gov/Star.
[4] M. Durante, F.A. Cucinotta, Physical basis of radiation protection in space travel. Rev. Mod. Phy. 83, 1245, 2011.
[5] D. Heynderickx, B. Quaghebeur, J. Wera, E. J. Daly, H. D. R. Evans, New radiation environment and effects models in ESA's space environment information system (SPENVIS) . Proceedings of the 7th European Conference on Radiation and Its Effects on Components and Systems, RADECS 2003.
[6] A. Ivantchenko, P. Nieminen, S. Incerti, G. Santin, V. Ivantchenko, V. Grichine, J. Allison, 40th COSPAR Scientific Assembly. Held 2-10 August 2014, in Moscow, Russia, Abstract F2.2-38-14, 2014.
[7] F. Lei, P. R. Truscott, C. S. Dyer, B. Quaghebeur, D. Heynderickx, P. Nieminen, H. Evans, E. Daly, MULASSIS: A Geant4-Based Multilayered Shielding Simulation Tool, IEEE Trans. Nucl. Sci. 49 (6), 2788–2793, 2003.
[8] R. E. McGuire, T. T. von Rosenvinge, F. B. McDonald, The composition of solar energetic particles, Astrophysical Journal. 301, 938-961, 1986.
[9] P. R. Truscott, F. Lei, C. Dyer, B. Quaghebeur, D. Heyndericks, P. Nieminen, H. Evans, E. Daly, A. Mohammadzadeh, G. Hopkinson, MULASSIS - Monte Carlo Radiation Shielding Simulation for Space Applications Made Easy, European Space Components Information Exchange System, ESCIES, 2003.
[10] J. W. Wilson, F. F. Badavi, F. A. Cucinotta, J. L. Shinn, G. D. Badhhwar, R. Silberberg, C.H. Tsao, L. W. Townsend, R. K. Tripathi, HZETRN: Description of a Free-Space Ion and Nucleon Transport and Shielding Computer Program, NASA TP-3495, 1995.
[11] J. F. Ziegler, The Stopping of Energetic Light Ions in Elemental Matter HZETRN: Description of a Free-Space Ion and Nucleon Transport and Shielding Computer Program, NASA TP-3495, 1995.
Cite This Article
  • APA Style

    Filomena Loffredo, Mariagabriella Pugliese, Maria Quarto, Vincenzo Roca, Valerio Pisacane, et al. (2015). Validation of the Electromagnetic Physical Processes with Software SPENVIS. American Journal of Environmental Protection, 4(6), 275-278. https://doi.org/10.11648/j.ajep.20150406.12

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    ACS Style

    Filomena Loffredo; Mariagabriella Pugliese; Maria Quarto; Vincenzo Roca; Valerio Pisacane, et al. Validation of the Electromagnetic Physical Processes with Software SPENVIS. Am. J. Environ. Prot. 2015, 4(6), 275-278. doi: 10.11648/j.ajep.20150406.12

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    AMA Style

    Filomena Loffredo, Mariagabriella Pugliese, Maria Quarto, Vincenzo Roca, Valerio Pisacane, et al. Validation of the Electromagnetic Physical Processes with Software SPENVIS. Am J Environ Prot. 2015;4(6):275-278. doi: 10.11648/j.ajep.20150406.12

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  • @article{10.11648/j.ajep.20150406.12,
      author = {Filomena Loffredo and Mariagabriella Pugliese and Maria Quarto and Vincenzo Roca and Valerio Pisacane and Renato Aurigemma},
      title = {Validation of the Electromagnetic Physical Processes with Software SPENVIS},
      journal = {American Journal of Environmental Protection},
      volume = {4},
      number = {6},
      pages = {275-278},
      doi = {10.11648/j.ajep.20150406.12},
      url = {https://doi.org/10.11648/j.ajep.20150406.12},
      eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajep.20150406.12},
      abstract = {The Space Radiation represents a serious risk for astronauts during space missions. The risk related to the space radiation exposure could involve acute and/or late effects. The Solar Cosmic Radiation that consists of protons (≈98%) with a very wide spectrum in energy (up to several GeV), is the major source of exposure for the crew. In this paper we present the results of the validation of the electromagnetic physical processes with the aim to contribute to the study of radiation protection for astronauts, in particular against the radiation due to the Solar Particle Events (SPE). The simulation was performed using MULASSIS, a module to the software SPENVIS, with protons as source, in the energy range from 800 MeV to 1.2 GeV, on a slab of aluminum of mass thickness of 20 g/cm2. The results obtained by the simulation were compared with PSTAR database of the NIST. Finally, a comparison between SPENVIS and Geant4-9.6p2 was performed.},
     year = {2015}
    }
    

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    AU  - Filomena Loffredo
    AU  - Mariagabriella Pugliese
    AU  - Maria Quarto
    AU  - Vincenzo Roca
    AU  - Valerio Pisacane
    AU  - Renato Aurigemma
    Y1  - 2015/10/27
    PY  - 2015
    N1  - https://doi.org/10.11648/j.ajep.20150406.12
    DO  - 10.11648/j.ajep.20150406.12
    T2  - American Journal of Environmental Protection
    JF  - American Journal of Environmental Protection
    JO  - American Journal of Environmental Protection
    SP  - 275
    EP  - 278
    PB  - Science Publishing Group
    SN  - 2328-5699
    UR  - https://doi.org/10.11648/j.ajep.20150406.12
    AB  - The Space Radiation represents a serious risk for astronauts during space missions. The risk related to the space radiation exposure could involve acute and/or late effects. The Solar Cosmic Radiation that consists of protons (≈98%) with a very wide spectrum in energy (up to several GeV), is the major source of exposure for the crew. In this paper we present the results of the validation of the electromagnetic physical processes with the aim to contribute to the study of radiation protection for astronauts, in particular against the radiation due to the Solar Particle Events (SPE). The simulation was performed using MULASSIS, a module to the software SPENVIS, with protons as source, in the energy range from 800 MeV to 1.2 GeV, on a slab of aluminum of mass thickness of 20 g/cm2. The results obtained by the simulation were compared with PSTAR database of the NIST. Finally, a comparison between SPENVIS and Geant4-9.6p2 was performed.
    VL  - 4
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    ER  - 

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Author Information
  • Dipartimento di Fisica, Università di Napoli Federico II, Naples, Italy

  • Dipartimento di Fisica, Università di Napoli Federico II, Naples, Italy

  • Dipartimento di Fisica, Università di Napoli Federico II, Naples, Italy

  • Dipartimento di Fisica, Università di Napoli Federico II, Naples, Italy

  • Euro.Soft srl, Naples, Italy

  • Consorzio Società Aerospaziale Mediterranea (SAM), Naples, Italy

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